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IIT JEE Physics Practice Paper – Gravitation (Set 25)

IIT JEE Physics Practice Paper – Gravitation (Set 25)

Instructions

Total Questions: 20 | Marks: 4 each | No Negative Marking

Q1. Newton’s law of gravitation states force is proportional to:




Q2. Gravitational force inversely depends on:




Q3. Universal gravitational constant symbol:




Q4. SI unit of gravitational constant:




Q5. Acceleration due to gravity on Earth is nearly:




Q6. Value of g decreases with:




Q7. Escape velocity from Earth surface is approximately:




Q8. Escape velocity formula:




Q9. Orbital velocity of satellite depends on:




Q10. Orbital velocity formula:




Q11. Geostationary satellite period is:




Q12. Weight of body at Earth center is:




Q13. Gravitational potential energy formula:




Q14. Gravitational field intensity unit:




Q15. Kepler’s first law states planets move in:




Q16. Kepler’s second law is law of:




Q17. Kepler’s third law relation:




Q18. Weightlessness in satellite is due to:




Q19. Gravitational force is always:




Q20. Relation between g and G:




Gravitation – IIT JEE Notes (Set 25)

Introduction to Gravitation

Definition

Gravitation is the universal force of attraction between any two masses in the universe.

Importance

It explains planetary motion, satellite motion, tides, and falling of bodies toward Earth.

Newton’s Law of Gravitation

Statement

Every particle attracts every other particle with a force directly proportional to product of their masses and inversely proportional to square of distance between them.

Formula

F = Gm₁m₂/r²

Variables

F = gravitational force

G = universal gravitational constant

m₁, m₂ = masses

r = separation between centers

Universal Gravitational Constant

Symbol

G

Value

G = 6.67 × 10⁻¹¹ Nm²/kg²

Importance

Its value remains same everywhere in the universe.

Characteristics of Gravitational Force

Main Features

Always attractive, central in nature, long range force, and obeys inverse square law.

Weak Force

Gravitational force is weakest among fundamental forces.

Acceleration Due to Gravity

Definition

Acceleration produced in a body due to Earth’s gravitational pull.

Formula

g = GM/R²

Standard Value

g ≈ 9.8 m/s²

Variation of g with Height

Relation

Acceleration due to gravity decreases with increase in height above Earth surface.

Approximate Formula

gh = g(1 – 2h/R)

Variation of g with Depth

Relation

Acceleration due to gravity decreases with depth below Earth surface.

Formula

gd = g(1 – d/R)

Important Point

g becomes zero at center of Earth.

Variation of g Due to Earth Rotation

Effect

g is maximum at poles and minimum at equator.

Reason

Centrifugal force due to Earth rotation reduces effective gravity at equator.

Mass and Weight

Mass

Amount of matter in a body and remains constant everywhere.

Weight

Force with which Earth attracts a body.

Formula

W = mg

Key Insight

Weight changes from place to place while mass remains constant.

Gravitational Potential

Definition

Work done per unit mass in bringing a body from infinity to a point.

Formula

V = -GM/r

Unit

J/kg

Gravitational Potential Energy

Definition

Energy possessed by a body due to gravitational interaction.

Formula

U = -GMm/r

Important Point

Potential energy is negative because gravitational force is attractive.

Escape Velocity

Definition

Minimum velocity required for a body to escape Earth’s gravitational field permanently.

Formula

ve = √(2GM/R)

Value for Earth

Approximately 11.2 km/s.

Important Point

Escape velocity is independent of mass of body.

Orbital Velocity

Definition

Velocity required for satellite to remain in stable orbit around Earth.

Formula

v = √(GM/R)

Value Near Earth

Approximately 7.9 km/s.

Satellites

Definition

Objects revolving around planets under gravitational attraction.

Natural Satellites

Moon is natural satellite of Earth.

Artificial Satellites

Man-made satellites used for communication, weather, and navigation.

Geostationary Satellite

Definition

Satellite appearing stationary relative to Earth.

Conditions

Orbital period must be 24 hours and orbit must lie in equatorial plane.

Applications

Communication and weather forecasting.

Kepler’s Laws of Planetary Motion

First Law

Planets move in elliptical orbits with Sun at one focus.

Second Law

Line joining Sun and planet sweeps equal areas in equal intervals of time.

Third Law

Square of orbital period is proportional to cube of semi-major axis.

T² ∝ R³

Weightlessness

Definition

Condition when apparent weight becomes zero.

Cause in Satellites

Satellites and astronauts remain in continuous free fall.

Energy of Satellite

Kinetic Energy

K = GMm/2R

Potential Energy

U = -GMm/R

Total Energy

E = -GMm/2R

Gravitational Field Intensity

Definition

Force experienced by unit mass placed at a point.

Formula

E = GM/r²

Unit

N/kg

Tides

Cause

Tides are caused mainly due to gravitational pull of Moon and Sun.

Types

High tide and low tide.

Conceptual Insights

Key Understanding

Gravitational force governs motion of celestial bodies and keeps planets and satellites in orbit.

Common Mistakes

Students often confuse orbital velocity with escape velocity and misuse signs in gravitational potential energy.

Important Exam Concepts

Conceptual Traps

Escape velocity is √2 times orbital velocity near Earth surface.

JEE Strategy

Practice derivations, satellite motion numericals, Kepler’s laws, and variation of g thoroughly for IIT JEE preparation.

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